English

Kinetically Driven Quintessence

Astrophysics 2008-11-26 v2 High Energy Physics - Phenomenology

Abstract

Recently, a novel class of models for inflation has been found in which the inflationary dynamics is driven solely by (non-canonical) kinetic terms rather than by potential terms. As an obvious extension, we show that a scalar field with non-canonical kinetic terms alone behaves like an energy component which is time-varying and has negative pressure presently, i.e. quintessence. We present a model which has a constant equation of state, that is, a ``kinetic'' counterpart of the Ratra-Peebles model of a quintessence field with a potential term. We make clear the structure of the phase plane and show that the quintessential solution is a late-time attractor. We also give a model for the ``phantom'' component which has an equation of state with w=p/ρ<1w=p/\rho <-1.

Keywords

Cite

@article{arxiv.astro-ph/9912463,
  title  = {Kinetically Driven Quintessence},
  author = {Takeshi Chiba and Takahiro Okabe and Masahide Yamaguchi},
  journal= {arXiv preprint arXiv:astro-ph/9912463},
  year   = {2008}
}

Comments

18 pages, minor changes, to be published in Physical Review D